The following chart shows the position where the Moon
is directly overhead at the maximum times of the
total (in blue) and
partial (in red) lunar eclipses (penumbral eclipses are
omitted). Each eclipse will be visible approximately
from the half of the Earth centred on that point. Note
that we only have mapping data for
eclipses from year 1 AD, so any eclipses prior to that
date will be missing. Use the
zoom controls on the left to zoom in and out; hover over
a marker to see the area of visibility and summary
information on that eclipse.
The interactive map is currently not available.
13 Apr, 1680 AD
max: 23:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.06; Saros 136)
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In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 6% of the Moon's disc for 1 hour and 14 minutes, which was essentially impossible to see.
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25 Apr, 1698 AD
max: 06:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.17; Saros 136)
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In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 17% of the Moon's disc for 2 hours and 6 minutes, which was essentially impossible to see.
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6 May, 1716 AD
max: 12:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.29; Saros 136)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 44 minutes, just 29% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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17 May, 1734 AD
max: 19:38 UT
Penumbral Lunar Eclipse
(penum. mag. 0.43; Saros 136)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 15 minutes, just 43% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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28 May, 1752 AD
max: 02:13 UT
Penumbral Lunar Eclipse
(penum. mag. 0.57; Saros 136)
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This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 42 minutes, just 57% of the Moon's disc was in partial shadow (with no part of it in complete shadow).
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8 Jun, 1770 AD
max: 08:44 UT
Penumbral Lunar Eclipse
(penum. mag. 0.72; Saros 136)
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This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 72% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 5 minutes.
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18 Jun, 1788 AD
max: 15:15 UT
Penumbral Lunar Eclipse
(penum. mag. 0.87; Saros 136)
|
This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 87% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 26 minutes.
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30 Jun, 1806 AD
max: 21:44 UT
Penumbral Lunar Eclipse
(penum. mag. 1.03; Saros 136)
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In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth (though none of it was in complete shadow), and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 44 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
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11 Jul, 1824 AD
max: 04:14 UT
Partial Lunar Eclipse
(umbral mag. 0.13; Saros 136)
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At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 28 minutes, with just 13% of the Moon in shadow at maximum.
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22 Jul, 1842 AD
max: 10:47 UT
Partial Lunar Eclipse
(umbral mag. 0.29; Saros 136)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 29% of the Moon in shadow; the partial eclipse lasted for 2 hours and 7 minutes.
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1 Aug, 1860 AD
max: 17:24 UT
Partial Lunar Eclipse
(umbral mag. 0.45; Saros 136)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 45% of the Moon in shadow; the partial eclipse lasted for 2 hours and 32 minutes.
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13 Aug, 1878 AD
max: 00:08 UT
Partial Lunar Eclipse
(umbral mag. 0.59; Saros 136)
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The Earth's shadow on the moon was clearly visible in this eclipse, with 59% of the Moon in shadow; the partial eclipse lasted for 2 hours and 51 minutes.
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23 Aug, 1896 AD
max: 06:57 UT
Partial Lunar Eclipse
(umbral mag. 0.73; Saros 136)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 5 minutes, with 73% of the Moon in darkness at maximum.
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4 Sep, 1914 AD
max: 13:54 UT
Partial Lunar Eclipse
(umbral mag. 0.86; Saros 136)
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The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 16 minutes, with 86% of the Moon in darkness at maximum.
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14 Sep, 1932 AD
max: 21:00 UT
Partial Lunar Eclipse
(umbral mag. 0.98; Saros 136)
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The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 24 minutes. With 98% of the Moon in shadow at maximum eclipse, this was quite a memorable event.
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26 Sep, 1950 AD
max: 04:16 UT
Total Lunar Eclipse
(umbral mag. 1.08; Saros 136)
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A shallow total eclipse saw the Moon in relative darkness for 44 minutes and 18 seconds. The Moon was 8% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 30 minutes in total.
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6 Oct, 1968 AD
max: 11:41 UT
Total Lunar Eclipse
(umbral mag. 1.17; Saros 136)
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A shallow total eclipse saw the Moon in relative darkness for 1 hour and 3 minutes. The Moon was 17% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 34 minutes in total.
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17 Oct, 1986 AD
max: 19:17 UT
Total Lunar Eclipse
(umbral mag. 1.25; Saros 136)
|
The Moon was plunged into darkness for 1 hour and 14 minutes, in a deep total eclipse which saw the Moon 25% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours and 37 minutes in total.
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28 Oct, 2004 AD
00:07–06:01 UT
Total Lunar Eclipse
(umbral mag. 1.31; Saros 136)
|
The Moon was plunged into darkness for 1 hour and 21 minutes, in a deep total eclipse which saw the Moon 31% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour for observers over the Americas, Europe, Africa, and parts of Asia. The partial eclipse lasted for 3 hours and 39 minutes in total.
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8 Nov, 2022 AD
08:02–13:56 UT
Total Lunar Eclipse
(umbral mag. 1.36; Saros 136)
|
The Moon was plunged into darkness for 1 hour and 25 minutes, in a deep total eclipse which saw the Moon 36% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour for observers from most of Asia, Australia, the Pacific, and North and Central America. The partial eclipse lasted for 3 hours and 40 minutes in total.
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18 Nov, 2040 AD
16:06–22:00 UT
Total Lunar Eclipse
(umbral mag. 1.40; Saros 136)
|
The Moon will be plunged into darkness for 1 hour and 28 minutes, in a deep total eclipse which will see the Moon 40% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour for observers from Europe, Asia, and Australia. The partial eclipse will last for 3 hours and 40 minutes in total.
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30 Nov, 2058 AD
max: 03:14 UT
Total Lunar Eclipse
(umbral mag. 1.43; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 30 minutes, in a deep total eclipse which will see the Moon 43% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 41 minutes in total.
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10 Dec, 2076 AD
max: 11:32 UT
Total Lunar Eclipse
(umbral mag. 1.45; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 31 minutes, in a deep total eclipse which will see the Moon 45% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 41 minutes in total.
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21 Dec, 2094 AD
max: 19:53 UT
Total Lunar Eclipse
(umbral mag. 1.46; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 32 minutes, in a deep total eclipse which will see the Moon 46% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 41 minutes in total.
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2 Jan, 2113 AD
max: 04:19 UT
Total Lunar Eclipse
(umbral mag. 1.47; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 32 minutes, in a deep total eclipse which will see the Moon 47% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 40 minutes in total.
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13 Jan, 2131 AD
max: 12:45 UT
Total Lunar Eclipse
(umbral mag. 1.48; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which will see the Moon 48% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 40 minutes in total.
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23 Jan, 2149 AD
max: 21:11 UT
Total Lunar Eclipse
(umbral mag. 1.50; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which will see the Moon 50% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 40 minutes in total.
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4 Feb, 2167 AD
max: 05:35 UT
Total Lunar Eclipse
(umbral mag. 1.51; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 34 minutes, in a deep total eclipse which will see the Moon 51% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 39 minutes in total.
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14 Feb, 2185 AD
max: 13:56 UT
Total Lunar Eclipse
(umbral mag. 1.54; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 35 minutes, in a deep total eclipse which will see the Moon 54% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 39 minutes in total.
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26 Feb, 2203 AD
max: 22:13 UT
Total Lunar Eclipse
(umbral mag. 1.57; Saros 136)
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A dramatic total eclipse lasting 1 hour and 36 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 40 minutes in total.
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9 Mar, 2221 AD
max: 06:24 UT
Total Lunar Eclipse
(umbral mag. 1.61; Saros 136)
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A dramatic total eclipse lasting 1 hour and 38 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 40 minutes in total.
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20 Mar, 2239 AD
max: 14:28 UT
Total Lunar Eclipse
(umbral mag. 1.66; Saros 136)
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A dramatic total eclipse lasting 1 hour and 39 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 40 minutes in total.
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30 Mar, 2257 AD
max: 22:26 UT
Total Lunar Eclipse
(umbral mag. 1.73; Saros 136)
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A dramatic total eclipse lasting 1 hour and 40 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 40 minutes in total.
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11 Apr, 2275 AD
max: 06:17 UT
Total Lunar Eclipse
(umbral mag. 1.80; Saros 136)
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A dramatic total eclipse lasting 1 hour and 41 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 40 minutes in total.
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21 Apr, 2293 AD
max: 14:01 UT
Total Lunar Eclipse
(umbral mag. 1.83; Saros 136)
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A dramatic total eclipse lasting 1 hour and 41 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 40 minutes in total.
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3 May, 2311 AD
max: 21:39 UT
Total Lunar Eclipse
(umbral mag. 1.73; Saros 136)
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A dramatic total eclipse lasting 1 hour and 40 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 39 minutes in total.
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14 May, 2329 AD
max: 05:12 UT
Total Lunar Eclipse
(umbral mag. 1.63; Saros 136)
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A dramatic total eclipse lasting 1 hour and 38 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 37 minutes in total.
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25 May, 2347 AD
max: 12:39 UT
Total Lunar Eclipse
(umbral mag. 1.52; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 33 minutes, in a deep total eclipse which will see the Moon 52% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 34 minutes in total.
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4 Jun, 2365 AD
max: 20:03 UT
Total Lunar Eclipse
(umbral mag. 1.40; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 25 minutes, in a deep total eclipse which will see the Moon 40% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 31 minutes in total.
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16 Jun, 2383 AD
max: 03:22 UT
Total Lunar Eclipse
(umbral mag. 1.27; Saros 136)
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The Moon will be plunged into darkness for 1 hour and 13 minutes, in a deep total eclipse which will see the Moon 27% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 26 minutes in total.
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26 Jun, 2401 AD
max: 10:42 UT
Total Lunar Eclipse
(umbral mag. 1.14; Saros 136)
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A shallow total eclipse will see the Moon in relative darkness for 54 minutes and 36 seconds. The Moon will be 14% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 19 minutes in total.
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7 Jul, 2419 AD
max: 17:58 UT
Total Lunar Eclipse
(umbral mag. 1.00; Saros 136)
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The Moon will barely edge into total eclipse for a brief 8 minutes and 36 seconds. With the Moon just barely inside the Earth's umbral shadow, the Moon may be quite bright, but even so, this should be worth seeing. The partial eclipse will last for 3 hours and 11 minutes in total.
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18 Jul, 2437 AD
max: 01:18 UT
Partial Lunar Eclipse
(umbral mag. 0.87; Saros 136)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 3 hours and 2 minutes, with 87% of the Moon in darkness at maximum.
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29 Jul, 2455 AD
max: 08:37 UT
Partial Lunar Eclipse
(umbral mag. 0.74; Saros 136)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 51 minutes, with 74% of the Moon in darkness at maximum.
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8 Aug, 2473 AD
max: 16:01 UT
Partial Lunar Eclipse
(umbral mag. 0.61; Saros 136)
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The Moon will be strikingly shadowed in this deep partial eclipse lasting 2 hours and 38 minutes, with 61% of the Moon in darkness at maximum.
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19 Aug, 2491 AD
max: 23:28 UT
Partial Lunar Eclipse
(umbral mag. 0.48; Saros 136)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 48% of the Moon in shadow; the partial eclipse will last for 2 hours and 24 minutes.
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31 Aug, 2509 AD
max: 07:02 UT
Partial Lunar Eclipse
(umbral mag. 0.37; Saros 136)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 37% of the Moon in shadow; the partial eclipse will last for 2 hours and 7 minutes.
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11 Sep, 2527 AD
max: 14:42 UT
Partial Lunar Eclipse
(umbral mag. 0.26; Saros 136)
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The Earth's shadow on the moon will be clearly visible in this eclipse, with 26% of the Moon in shadow; the partial eclipse will last for 1 hour and 48 minutes.
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21 Sep, 2545 AD
max: 22:28 UT
Partial Lunar Eclipse
(umbral mag. 0.16; Saros 136)
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At maximum eclipse, a small bite out of the Moon should be visible. The eclipse will last for 1 hour and 26 minutes, with just 16% of the Moon in shadow at maximum.
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3 Oct, 2563 AD
max: 06:22 UT
Partial Lunar Eclipse
(umbral mag. 0.07; Saros 136)
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A tiny bite out of the Moon may be visible at maximum, though just 7% of the Moon will be shadowed in a partial eclipse lasting for 58 minutes and 12 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.
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13 Oct, 2581 AD
max: 14:23 UT
Penumbral Lunar Eclipse
(penum. mag. 0.96; Saros 136)
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The Moon will approach within 1% of the Earth's umbral shadow at maximum eclipse; 96% of the Moon's disc will be partially shaded by the Earth, with the overall eclipse lasting 4 hours exactly. While less dramatic than a partial eclipse (as no part of the Moon will be in complete shadow), a shading across the Moon should be readily visible to observers.
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24 Oct, 2599 AD
max: 22:34 UT
Penumbral Lunar Eclipse
(penum. mag. 0.89; Saros 136)
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At maximum eclipse, 89% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 3 hours and 53 minutes overall.
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5 Nov, 2617 AD
max: 06:51 UT
Penumbral Lunar Eclipse
(penum. mag. 0.84; Saros 136)
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At maximum eclipse, 84% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 3 hours and 47 minutes overall.
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16 Nov, 2635 AD
max: 15:17 UT
Penumbral Lunar Eclipse
(penum. mag. 0.80; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 80% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 42 minutes.
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26 Nov, 2653 AD
max: 23:49 UT
Penumbral Lunar Eclipse
(penum. mag. 0.76; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 76% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 38 minutes.
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8 Dec, 2671 AD
max: 08:28 UT
Penumbral Lunar Eclipse
(penum. mag. 0.74; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 74% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 35 minutes.
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18 Dec, 2689 AD
max: 17:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.72; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 72% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 33 minutes.
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31 Dec, 2707 AD
max: 01:58 UT
Penumbral Lunar Eclipse
(penum. mag. 0.71; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 71% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 31 minutes.
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10 Jan, 2726 AD
max: 10:48 UT
Penumbral Lunar Eclipse
(penum. mag. 0.70; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 70% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 30 minutes.
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21 Jan, 2744 AD
max: 19:38 UT
Penumbral Lunar Eclipse
(penum. mag. 0.69; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 69% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 29 minutes.
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1 Feb, 2762 AD
max: 04:27 UT
Penumbral Lunar Eclipse
(penum. mag. 0.68; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 68% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 28 minutes.
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12 Feb, 2780 AD
max: 13:15 UT
Penumbral Lunar Eclipse
(penum. mag. 0.67; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 67% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 26 minutes.
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22 Feb, 2798 AD
max: 21:59 UT
Penumbral Lunar Eclipse
(penum. mag. 0.65; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 65% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 23 minutes.
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5 Mar, 2816 AD
max: 06:38 UT
Penumbral Lunar Eclipse
(penum. mag. 0.62; Saros 136)
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This subtle penumbral eclipse may be visible to a skilled observer at maximum eclipse. 62% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 20 minutes.
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16 Mar, 2834 AD
max: 15:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.59; Saros 136)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 14 minutes, just 59% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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26 Mar, 2852 AD
max: 23:38 UT
Penumbral Lunar Eclipse
(penum. mag. 0.54; Saros 136)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 8 minutes, just 54% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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7 Apr, 2870 AD
max: 07:57 UT
Penumbral Lunar Eclipse
(penum. mag. 0.48; Saros 136)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 58 minutes, just 48% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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17 Apr, 2888 AD
max: 16:08 UT
Penumbral Lunar Eclipse
(penum. mag. 0.41; Saros 136)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 46 minutes, just 41% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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30 Apr, 2906 AD
max: 00:11 UT
Penumbral Lunar Eclipse
(penum. mag. 0.33; Saros 136)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 30 minutes, just 33% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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10 May, 2924 AD
max: 08:07 UT
Penumbral Lunar Eclipse
(penum. mag. 0.24; Saros 136)
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This very subtle penumbral eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 10 minutes, just 24% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).
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21 May, 2942 AD
max: 15:54 UT
Penumbral Lunar Eclipse
(penum. mag. 0.14; Saros 136)
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In this extremely marginal eclipse, the Moon barely clips the edge of the Earth's penumbral shadow. This will cause a microscopic darkening of just 14% of the Moon's disc for 1 hour and 39 minutes, which will be essentially impossible to see.
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31 May, 2960 AD
max: 23:36 UT
Penumbral Lunar Eclipse
(penum. mag. 0.03; Saros 136)
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In this extremely marginal eclipse, the Moon barely clips the edge of the Earth's penumbral shadow. This will cause a microscopic darkening of just 3% of the Moon's disc for 46 minutes and 6 seconds, which will be essentially impossible to see.
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